Long wavelength cosmological surveys with ISO

Details Long wavelength cosmological surveys with ISO Long wavelength cosmological surveys with ISO

Mar 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999esasp.427.1007p&link_type=abstract

The Universe as Seen by ISO. Eds. P. Cox & M. F. Kessler. ESA-SP 427., p. 1007

Mathematics

Logic

1

Far-Infrared, Cosmology

Scientific paper

We review ISO deep surveys at wavelengths longer than 100 μm beyond which the redshift of the peak emission of starburst galaxies (at 60 to 80 μm) tends to favour distant sources. The number counts of sources at 175 μm show a very steep slope between 100 mJy and 1 Jy implying a strong cosmological evolution. It is also shown that deep surveys in low cirrus regions show the structure of the background with a large signal to noise ratio. The anisotropies of the background are dominated at angular scales close to the angular resolution by the structure of the extragalactic background which will, thus, be a very useful tool for cosmological studies until large passively cooled telescopes in space become available.

Affiliated with

Also associated with

No associations

Rating

Long wavelength cosmological surveys with ISO does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Long wavelength cosmological surveys with ISO, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Long wavelength cosmological surveys with ISO will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1447774